Ryu 517
Summary
Ryu 517 is a sparse, very dense object of low C3 quality. It is located at a moderate distance from the Sun, near the mid-plane. It is rarely studied in the literature, with no articles listed in the last 6 years.
This object shares a small percentage of members with at least one entry reported in the same catalogue.
Warning: contains less than 25 stars with P>0.5 estimated.
Positions
| Reference | RA | DEC | Plx | pmRA | pmDE | Rv |
|---|---|---|---|---|---|---|
| Bica et al. (2019) | 265.21 | -30.446 | – | – | – | – |
| UCC | 265.221 | -30.432 | 0.467 | 0.126 | -1.013 | – |
Estimated members
Explore data in Colab
Search coordinates in Bayestar19
Cluster region map
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| VVV 130 | 20.0 | 265.29 | -30.42 | 0.44 | -0.1 | -1.04 | – | 0.19 |